Loudzoo
- 43
- 0
Thats my simple question!
The discussion centers on whether longwave radiation, specifically infrared (IR) radiation, can effectively heat the oceans. Participants explore the mechanisms of heat transfer, the role of evaporation, and the implications of atmospheric back radiation on ocean temperatures. The conversation includes theoretical considerations and challenges related to experimental observations.
Participants express differing views on the effectiveness of IR radiation in heating the oceans, with no consensus reached. Some agree that IR contributes to surface heating but debate its overall impact on deeper ocean temperatures, while others challenge the assumptions underlying these claims.
Participants highlight the complexity of measuring the effects of IR radiation on ocean temperatures, noting the challenges of isolating variables such as evaporation and heat conduction. The discussion also reflects varying interpretations of scientific data and models related to radiation absorption in water.
This discussion may be of interest to those studying climatology, oceanography, or the effects of greenhouse gases on climate systems, as well as individuals curious about the interactions between radiation and oceanic processes.
Loudzoo said:IR does not penetrate below 1cm
... not "wrong," into a "semantic ditch," perhaps. If you're going to give me all the solar radiation that penetrates further than 1 mm by the Kebes plot (shorter than 2 μm), you've given me 80 - 90% of the IR. If you define IR as only that radiation that is absorbed in 1 mm or less, and ignore the 0.8 - 2 μm gap between visible and IR acknowledged by a specific argument, you're losing a lot of energy.Loudzoo said:Where am I going
What is "back radiation?"Loudzoo said:Can an increase in Atmospheric back radiation
Not being "flip" with you --- just wanted to be sure we're both working from the same initial set of ideas/postulates/principles.Loudzoo said:Heat moves from hot to cold obviously.
Welcome to the wonderful world of energy "balances" in non-equilibrium systems. The system we're "analyzing" (hah!) has as heat sources the sun, ~ 10-4steradians at ~ 5800 K or 1-1.3 kW/m2 at Earth surface, and crustal heat leak of 10-30 mW/m2, negligible. The heat sink is 4π steradians at ~ 4 K, the CMB. What else do we know? Some fraction of incident solar radiation is reflected, what fraction is subject to some uncertainty; some fraction is transmitted, very small through the atmospheric "halo", but enough to illuminate an otherwise totally eclipsed moon; and, some fraction is absorbed by atmo-, hydro-, and lithospheres, exchanged by conduction, convection, and radiation, and radiated to the CMB.Loudzoo said:And quite frankly I'm confused!
Loudzoo said:I understand the popular theory well enough but I don't understand the physical process of how additional CO2 in the atmosphere can lead to higher ocean temperatures. Can you help me?